Life on Europa?

This moon of Jupiter might have life in a subsurface ocean.

Life on Europa: Water from a subsurface ocean on Jupiter's moon, Europa, could reach the surface through seeps or erupt from hot water vents. This water would reveal the chemistry of the subsurface ocean and may contain microbes that live below. Artist's concept image by NASA / JPL.

Subsurface structure of Europa: This image shows the internal structure of Europa. It has an icy crust supported by a subsurface ocean. Below that is the rocky layer surrounding an iron core. Image by NASA / JPL.

The New Search for Extraterrestrial Life

For the past several centuries, everyone believed that Mars was the most likely body in our solar system to support
life beyond Earth. But after centuries of telescope observation, decades of spacecraft exploration, and several
robots exploring its surface, the promise of discovering life on Mars remains elusive.

Now, scientific attention is being focused on Europa, the fourth-largest of Jupiter's 67 confirmed moons. It may be
an even better candidate for finding life than Mars. For life to be present the three basic requirements are: 1) liquid
water; 2) chemical building blocks; and, 3) a source of energy. Europa is thought to have all three.

1) Europa's Liquid Water

The surface of Europa is very cold and covered with ice. This ice forms a "crust" on the moon that is thought to
be several kilometers thick. Beneath the crust, a subsurface ocean of liquid water up to 100 kilometers deep is thought
to exist. Investigators believe that the ocean is rich in dissolved ions, particularly magnesium, sodium, potassium,
and chlorine. Organisms on Earth live in ion-rich solutions, so there is a good chance that they live in them on Europa.

2) Europa's Building Blocks of Life

Spacecraft observations determined that the surface of Europa is covered with water ice. That ice and other materials on
Europa's surface are bombarded with radiation from Jupiter that could alter them into some of the chemical building blocks
of life. These include: free oxygen (O2), hydrogen peroxide (H2O2), carbon dioxide
(CO2), and sulfur dioxide (SO2).

If these compounds reach the subsurface ocean, they can be valuable nutrients to start and sustain life. The ocean water
can react with the rocks and minerals of the subsurface ocean's floor to liberate other nutrients to support life.

Video: The Europa-Jupiter System Mission, produced by NASA / JPL News.

3) Europa's Energy Source

Europa's position in space is within the powerful gravitational field of Jupiter. This strong gravitational "pull" has the
moon locked into an orbit with one hemisphere constantly facing Jupiter. The elliptical orbit takes Europa alternatively closer to and
farther away from the planet. This alternating increase and decrease of gravitational force on Europa results in the moon
elongating and relaxing with each trip around the planet. This internal movement, combined with gravitational forces exerted by neighboring
moons, produces internal friction and heat within Europa.

Europa's internal heat could be the energy source that keeps the subsurface ocean from freezing and sustains any life that
exists there. There could be hot water vents on the floor of the subsurface ocean that deliver energy and nutrients from the
planet's interior. Organisms on Earth have been discovered in the subglacial lakes of Antarctica and in the hot ion-rich
waters of hydrothermal vents. Life in Europa's subsurface oceans could be supported in similar ways.

Europa from Galileo: An image of the trailing hemisphere of Europa. It shows very few impact structures but numerous ridges and fractures
that suggest a rigid crust moving over a mobile layer below. Image by NASA.

Evidence for the Subsurface Ocean

NASA gives three pieces of evidence that strongly support the presence of Europa's subsurface ocean.

1) Magnetometer surveys done by the Galileo spacecraft discovered an induced magnetic field near Europa's surface.
This suggests a large body of conductive material (salty water) at a depth of 30 kilometers (about 20 miles) or less.

2) The surface of Europa has bands, ridges, fractures and multi-ringed impact structures that suggest
the presence of mobile material below.

3) The surface of Europa has large-scale fractures and ridges similar to those that bound Earth's tectonic plates. These
suggest a mobile layer below Europa's crust that supports the crust and allows it to move.

Life on Europa Might be Easy to Find

The presence of magnesium compounds on the surface of Europa suggests that water from the subsurface ocean reaches
the surface through springs or vents. If this occurs these eruptions would deliver up ions and microbes from the ocean below.

So, if there is life in Europa's subsurface ocean, it could be scattered about the surface of the planet where landers or rovers
might find it. A mission to the surface of the Europa might easily find evidence of life or even some of the microbes by
sampling surface materials.

This makes Europa a very interesting target in the search for extraterrestrial life. Some researchers believe that
it is a much better target than Mars.